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The BOSS bispectrum analysis at one loop from the Effective Field Theory of Large-Scale Structure

Guido D’AmicoDepartment of Mathematical, Physical and Computer Sciences, University of Parma, 43124 Parma, ItalyYaniv DonathDepartment of Applied Mathematics and Theoretical Physics, University of Cambridge, Cambridge, CB3 OWA, U.KMatthew LewandowskiDepartment of Physics and Astronomy, Northwestern University, Evanston, IL 60208, U.S.ALeonardo SenatoreInstitut fur Theoretische Physik, ETH Zurich, 8093 Zurich, SwitzerlandPierre ZhangCAS Key Laboratory for Research in Galaxies and Cosmology, University of Science and Technology of China, Hefei, Anhui 230026, China
2024en
ABI

Аннотация

Abstract We analyze the BOSS power spectrum monopole and quadrupole, and the bispectrum monopole and quadrupole data, using the predictions from the Effective Field Theory of Large-Scale Structure (EFTofLSS). Specifically, we use the one loop prediction for the power spectrum and the bispectrum monopole, and the tree level for the bispectrum quadrupole. After validating our pipeline against numerical simulations as well as checking for several internal consistencies, we apply it to the observational data. We find that analyzing the bispectrum monopole to higher wavenumbers thanks to the one-loop prediction, as well as the addition of the tree-level quadrupole, significantly reduces the error bars with respect to our original analysis of the power spectrum at one loop and bispectrum monopole at tree level. After fixing the spectral tilt to Planck preferred value and using a Big Bang Nucleosynthesis prior, we measure σ 8 = 0.794 ± 0.037, h = 0.692 ± 0.011, and Ω m = 0.311 ± 0.010 to about 4.7%, 1.6%, and 3.2%, at 68% CL, respectively. This represents an error bar reduction with respect to the power spectrum-only analysis of about 30%, 18%, and 13% respectively. Remarkably, the results are compatible with the ones obtained with a power-spectrum-only analysis, showing the power of the EFTofLSS in simultaneously predicting several observables. We find no tension with Planck.

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